Subjects: Astronomy >> Astrophysical processes submitted time 2023-10-23 Cooperative journals: 《天文研究与技术》
Abstract： The 1 m New Vacuum Solar Telescope (NVST) is capable of high-resolution imaging observations better than 0.2″, but cannot yet routinely observe high-resolution magnetic fields. Many magnetic structures and solar activity exist at small scales, requiring high-resolution magnetic field observations. NVST offers excellent seeing, and if the magnetometer has fast modulation capabilities and is coupled with statistical reconstruction techniques, it is expected to achieve high-resolution solar magnetic field measurements. The main problems faced by NVST in measuring magnetic fields include time-varying polarisation due to bending-axis optical paths, optical axis shifts due to telescope attitude changes and wind loading, and the effects of turbulence. In this paper, we analyze in detail the requirements for high-resolution observation of the solar magnetic field and the solar magnetic field measurement problems faced by NVST, formulate the basic parameters of the magnetometer, propose the requirements for the polarisation analyzer, and design a high-resolution observation scheme for the photospheric magnetic field. Finally, the optical path for the magnetometer is designed using ZEMAX optical design software, and the results show that the optical design can meet the requirements of high-resolution imaging.
Subjects: Astronomy >> Astrophysical processes submitted time 2023-10-23 Cooperative journals: 《天文研究与技术》
Abstract： The magnetic imager of ground-based solar telescope will be affected by atmospheric turbulence during polarimetry, resulting in inaccurate measurement results. By synchronously detecting the wavefront aberration, and to use deconvolution reconstruction of the sun′s narrow band polarization image, the poor photons problem caused by the narrow band filter can be overcome. The high-resolution image reconstruction algorithm is applied to the reconstruction of the sun′s polarized image. During the reconstruction process, inaccurate wavefront sensing result can lead to I crosstalk between the reconstructed polarization image and the real polarization signal, resulting in certain difference. To study the impact of wavefront sensing accuracy on polarization image reconstruction accuracy during the reduction, a simulation model is established in this paper to study the I crosstalk of polarimetry results under different seeing and wavefront sensing accuracy. The results indicate that the reconstruction quality of polarized images is positively correlated with the accuracy of wavefront sensing. Under certain conditions, increasing the number of frames used for image reconstruction and reducing image resolution can also reduce the I→QUV crosstalk.
Subjects: Astronomy >> Astrophysical processes submitted time 2020-05-06 Cooperative journals: 《天文研究与技术》
Abstract： 为充分利用丽江2.4米望远镜有限的卡焦接口，提高观测效率，研制了一个双视场天文观测终端，在2.4米望远镜上实现不同视场和图像比例尺等参数，进行快速测光和高分辨成像等天文观测，以满足天文学家的不同观测需求。针对该终端对滤光片轮精度和大视场光路与小视场光路切换的精度要求，以及对EMCCD相机图像采集的速度要求，本文采用三层电机闭环控制以及多线程并发执行等技术，实现了该终端中滤光片轮、大视场光路与小视场光路切换的精确控制，以及EMCCD相机图像的快速采集与存储。最后在实验室进行了详细测试，结果表明所设计的控制与图像采集能满足该终端的各项性能指标和功能指标的要求。
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